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The spectrum of the slowly varying component of solar radio emission at wavelengths of 3.3 mm – 21 cm

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Abstract

The spectrum and diameter of the source of the S-component emission (McMath Plage No. 244) observed on March 4, 1968 has been investigated at 3.3 mm, 4.3 mm, 8.5 mm, 2 cm, 9.1 cm, 21 cm, and 43 cm wavelengths.

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References

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Authors and Affiliations

  1. National Radio Astronomy Observatory, Green Bank, W.Va., U.S.A.

    A. Tlamicha

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  1. A. Tlamicha
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On leave of absence from the Astronomical Institute of the Czechoslovak Academy of Sciences, Observatory Ondfejov, Czechoslovakia.

Operated by Associated Universities, Inc., under contract with the National Science Foundation.

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Tlamicha, A. The spectrum of the slowly varying component of solar radio emission at wavelengths of 3.3 mm – 21 cm. Sol Phys 5, 377–381 (1968). https://doi.org/10.1007/BF00147151

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  • DOI: https://doi.org/10.1007/BF00147151

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